1. A new underground laboratory at Frejus Jacques Bouchez CEA-SACLAY NNN05-Aussois April 7, 2005 Historical overview Latest developments Outlook

2. PROTON DRIVER FOR CERN NEUTRINO FACTORY

3. Frejus lab is 130 km away from CERN ! E  = 270 MeV => baseline 135 km

5. A SAFETY GALLERY TO BE BUILT ALONG THE EXISTING TUNNEL

6. PROPOSAL FOR A NEW UNDERGROUND LAB AT FREJUS Excavation of safety gallery completed around 2009 when machines meet at the center. Excellent opportunity to dig a new cavity at reduced cost in the middle of the tunnel, which could be ready by 2012 and house a detector for the neutrino superbeam Horizontal access, rock quality known and good (and no water!) Schedule of such a detector comes much after T2K phase 1 and NuMI off-axis (now NOVA). So, directly propose a detector able to see CP violation => Megaton Cerenkov detector (or liquid Ar) First studies based on a UNO-like detector show excellent sensitivity to θ 13 and δ CP, similar to T2K phase 2 (4 MW + HK) Project favourably considered by our scientific authorities, with a strong support from local authorities

7. MORE RECENT DEVELOPMENTS A new idea (P.Zucchelli): Beta beams, produced by radioactive ions stored in a decay ring, give a novel way to produce e and anti- e beams of very high purity, perfectly known spectrum and intensity. The required ion energy is achievable with the SPS ! (see M.Lindroos’talk tomorrow) The combination of beta beams and superbeams gives unique redundancy (CP,T,CPT in different ways), and a direct handle on how the detector sees the signal in each beam (as it is the bulk of events seen with the other beam) The superbeam has been further optimized (higher energy, higher intensity) see M.Mezzetto’s talk tomorrow on the remarkable performances of Beta beams + superbeams. Beta beams profit from a strong synergy with nuclear physicists using radioactive ions produced by the ISOL technique: Neutrino beta beams are now part of the design study funded by Europe on the EURISOL facility.

8. EXCLUDED BY CHOOZ 1 5 9 Θ 13 degrees YEAR 06 12 1824 Minos, Icarus, Opera Double Chooz T2K1, NovA SB  B T2K 2

9. SCHEDULE Super and beta beams will hopefully be ready before 2020…. ….BUT We do not have to wait for them to build a detector, as non- accelerator physics is at least as rich as neutrino beam physics: proton decay, with some chance of discovery SN explosion ( for SN mechanism AND neutrino oscillations) So, our preferred strategy is: 1.Build a cavity and a detector, taking benefit of the safety gallery 2.Start non-accelerator physics right away 3.Begin neutrino oscillation study as soon as beams are available

10. A possibly optimistic schedule for a european lab. at Frejus Year 2005 09 2010 2015 2020 Safety tunnel Excavation Lab cavity Excavation P.S Study detector PM R&DPMT production Det.preparation InstallationOutside lab. Non-acc.physics P-decay, SN Superbeam ConstructionSuperbeam betabeam ???????? Beta beam Several modules: physics can start when the 1 st is ready

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12. Perlite insulation  ≈70 m h =20 m Electronic crates 100 kt liquid argon (see A. Rubbia’s talk)

13. FROM DREAM TO REALITY 1.A prestudy on the feasibility of the cavity has been launched: It will address maximal dimensions, preferred topology, cost… (both for Cerenkov and LAr): first results (very preliminary) will be presented by M.Levy on Saturday morning 2. Funding for a more detailed study will be requested to Europe in 2007 (next call) 3. R&D on photodetection is mandatory, a collaboration with Photonis has started. Other ideas on low cost large area photodetection (micromegas) are also considered. 4. We are looking forward to a closer inter-regional (north- America, Japan, Europe) cooperation, demonstrating a strong and converging interest on this very fundamental and promising field of physics

14. The end … of the prologue